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相关论文: Rotation of galaxies and dark matter

200 篇论文

The density profiles of dark halos are usually inferred from the rotation curves of disk galaxies based on the assumption that the gas is a good tracer of the gravitational potential of the galaxies. Some authors have suggested that…

天体物理学 · 物理学 2009-11-10 F. J. Sanchez-Salcedo , M. Reyes-Ruiz

Frankel et al (2020) reported that the rate of diffusion in angular momentum by stars in the disk of the Milky Way was about ten times faster than the rate of heating, which places a stringent requirement on the nature of disk star…

星系天体物理 · 物理学 2025-01-31 J A Sellwood , J Binney

We present a bi-metric theory of gravity containing a length scale of galactic size. For distances less than this scale the theory satisfies the standard tests of General Relativity. For distances greater than this scale the theory yields…

天体物理学 · 物理学 2009-10-31 I. T. Drummond

We present a study of the Milky Way disk and halo magnetic field, determined from observations of Faraday rotation measure (RM) towards 641 polarized extragalactic radio sources in the Galactic longitude range 100-117 degs, within 30 degs…

An axially symmetric galactic gravitational model composed of a dense, massive and spherical nucleus with an additional dark matter halo component was used, to distinguish between the regular and chaotic character of orbits of stars that…

星系天体物理 · 物理学 2017-09-28 Euaggelos E. Zotos , Nicolaos D. Caranicolas

The parameters of an axisymmetric model for the gravitational potential of the Galaxy have been refined. The basic curve of the Galaxy's rotation in a distance interval of $R:0-190$ kpc was constructed using the velocities of masers,…

星系天体物理 · 物理学 2026-01-14 V. V. Bobylev , A. T. Bajkova , A. A. Smirnov

The severity of the mass discrepancy in spiral galaxies is strongly correlated with the central surface brightness of the disk. Progressively lower surface brightness galaxies have ever larger mass discrepancies. No other parameter…

天体物理学 · 物理学 2015-06-24 Stacy McGaugh , Erwin de Blok

An study of the equatorial circular motion of photons and massive particles around a rotating compact body like a neutron star is presented. For this goal, we use an approximate Kerr-like metric with mass quadrupole as perturbation. The…

广义相对论与量子宇宙学 · 物理学 2024-05-01 Diego Solano-Alfaro , Francisco Frutos-Alfaro

A Faraday rotation experiment can set limits on the magnetic moment of a electrically-neutral, dark-matter particle, and the limits increase in stringency as the candidate-particle mass decreases. Consequently, if we assume the dark-matter…

高能物理 - 唯象学 · 物理学 2010-04-21 S. Gardner

If it is hypothesised that there is no dark matter then some alternative gravitational theory must take the place of general relativity (GR) on the largest scales. Dynamical measurements can be used to investigate the nature of such a…

天体物理学 · 物理学 2008-11-26 Daniel J. Mortlock , Edwin L. Turner

In the currently accepted paradigm, dark matter is hypothesized as an explanation of the flat rotation curves of galaxies under the assumption of virialized orbits. The use of millisecond pulsar timing as a probe of Galactic dark matter…

星系天体物理 · 物理学 2021-04-21 Kiley Heflin , Richard Lieu

In general relativity, the tangential speed of objects in stable circular orbits is not uniquely described by the orbital radius and the mass present inside the orbital radius. This work presents a static, spherically symmetric spacetime…

广义相对论与量子宇宙学 · 物理学 2025-04-24 C. Mallary

In a significant recent paper A. Edery undertakes a new study of light deflection in generalizations of general relativity (GR). He claims to prove that any metric-based gravitational theory that proposes to explain the flat rotation curves…

天体物理学 · 物理学 2009-10-31 J. D. Bekenstein , M. Milgrom , R. H. Sanders

The gravity fields and rotation curves of whirlpool galaxies with thin disc distribution of material are calculated numerically. It is proved that the gravity field of mass thin disc distribution is greatly different from that of…

综合物理 · 物理学 2009-03-12 Mei Xiaochun , Xu Kuan , Yu Ping

The dark matter accretion theory (around a central body) of the author on the basis of his 5-dimensional Projective Unified Field Theory (PUFT) is applied to the orbital motion of stars around the center of the Galaxy. The departure of the…

广义相对论与量子宇宙学 · 物理学 2009-11-07 E. Schmutzer

The observation of the bending of light by mass, now known as gravitational lensing, was key in establishing general relativity as one of the pillars of modern physics. In the past couple of decades, there has been increasing interest in…

广义相对论与量子宇宙学 · 物理学 2022-07-20 Arthur B. Congdon , Savitri V. Iyer , Charles R. Keeton

The growth of a massive black hole will steepen the cold dark matter density at the center of a galaxy into a dense spike, enhancing the prospects for indirect detection. We study the impact of black hole spin on the density profile using…

宇宙学与河外天体物理 · 物理学 2018-01-10 Francesc Ferrer , Augusto Medeiros da Rosa , Clifford M. Will

Recent studies have thrown up a big enigma. On the one hand they point to satellite galaxies rotating faster than they should with the usual theory. On the other hand they also go against explanation of Newtonian gravity with dark matter.…

综合物理 · 物理学 2012-08-03 B. G. Sidharth

We consider the generation and evolution of quantum fluctuations of a massive nonsymmetric gravitational field (B-field) from inflationary epoch to matter era in the simplest variant of the nonsymmetric theory of gravitation (NGT), which…

天体物理学 · 物理学 2016-08-30 Tomislav Prokopec , Wessel Valkenburg

Millisecond pulsars, representing the older neutron star population, are believed to have undergone a prolonged period of dark matter accumulation, resulting in a higher dark matter content. Their extreme rotation makes them unique…

高能天体物理现象 · 物理学 2025-06-27 Lorenzo Cipriani , Edoardo Giangrandi , Violetta Sagun , Daniela D. Doneva , Stoytcho S. Yazadjiev